Abstract
We describe a simple implementation of black hole excision in numerical relativity. We apply this technique to a Schwarzschild black hole with octant symmetry in Eddington-Finkelstein coordinates and show how one can obtain accurate, long-term stable numerical evolutions.
- Received 6 September 2000
DOI:https://doi.org/10.1103/PhysRevD.63.104006
©2001 American Physical Society